Q-Chem 4.3 User’s Manual

10.8 Spin and Charge Densities at the Nuclei

Gaussian basis sets violate nuclear cusp conditions [492, 493, 494]. This may lead to large errors in wavefunction at nuclei, particularly for spin density calculations [495]. This problem can be alleviated by using an averaging operator that compute wavefunction density based on constraints that wavefunction must satisfy near Coulomb singularity [496, 497]. The derivation of operators is based on hyper virial theorem [498] and presented in Ref. Rassolov:1996b. Application to molecular spin densities for spin-polarized [497] and DFT [499] wavefunctions show considerable improvement over traditional delta function operator.

One of the simplest forms of such operators is based on the Gaussian weight function $\exp [-(Z/r_{0})^{2}(\ensuremath{\mathbf{r}}-\ensuremath{\mathbf{R}})^{2}]$ that samples the vicinity of a nucleus of charge $Z$ located at $\bf R$. The parameter $r_0$ has to be small enough to neglect two-electron contributions of the order $\mbox{${\cal {O}}({r_{0}^4})$}$ but large enough for meaningful averaging. The range of values between 0.15–0.3 a.u. is shown to be adequate, with final answer being relatively insensitive to the exact choice of $r_0$ [496, 497]. The value of $r_0$ is chosen by RC_R0 keyword in the units of 0.001 a.u. The averaging operators are implemented for single determinant Hartree-Fock and DFT, and correlated SSG wavefunctions. Spin and charge densities are printed for all nuclei in a molecule, including ghost atoms.


Determines the parameter in the Gaussian weight function used to smooth the density at the nuclei.







Corresponds the traditional delta function spin and charge densities


corresponding to $n\times 10^{-3}$ a.u.


We recommend value of 250 for a typical spit valence basis. For basis sets with increased flexibility in the nuclear vicinity the smaller values of $r_0$ also yield adequate spin density.